Is Radiation of Quantized Black Holes Observable?
arXiv:astro-ph/0604003 · doi:10.1142/S0218271807010730
Abstract
If primordial black holes (PBH) saturate the present upper limit on the dark matter density in our Solar system and if their radiation spectrum is discrete, the sensitivity of modern detectors is close to that necessary for detecting this radiation. This conclusion is not in conflict with the upper limits on the PBH evaporation rate.
6 pages, 1 figure (reproduced properly in pdf file)